git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@12699 f3b2605a-c512-4ea7-a41b-209d697bcdaa
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@ -283,9 +283,9 @@ for the NEB procedure.
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<P>The damped dynamics <A HREF = "min_style.html">minimizers</A>, such as <I>quickmin</I>
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<P>The damped dynamics <A HREF = "min_style.html">minimizers</A>, such as <I>quickmin</I>
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and <I>fire</I>), adjust the position and velocity of the atoms via an
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and <I>fire</I>), adjust the position and velocity of the atoms via an
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Euler integration step. Thus you must define an appropriate
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Euler integration step. Thus you must define an appropriate
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<A HREF = "timestep.html">timestep</A> to use with NEB. Using the same timestep
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<A HREF = "timestep.html">timestep</A> to use with NEB. As mentioned above, NEB
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that would be used for a dynamics <A HREF = "run.html">run</A> of your system is
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will often converge more quickly if you use a timestep about 10x
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advised.
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larger than you would normally use for dynamics simulations.
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</P>
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</P>
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<HR>
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<HR>
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@ -273,9 +273,9 @@ for the NEB procedure.
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The damped dynamics "minimizers"_min_style.html, such as {quickmin}
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The damped dynamics "minimizers"_min_style.html, such as {quickmin}
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and {fire}), adjust the position and velocity of the atoms via an
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and {fire}), adjust the position and velocity of the atoms via an
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Euler integration step. Thus you must define an appropriate
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Euler integration step. Thus you must define an appropriate
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"timestep"_timestep.html to use with NEB. Using the same timestep
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"timestep"_timestep.html to use with NEB. As mentioned above, NEB
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that would be used for a dynamics "run"_run.html of your system is
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will often converge more quickly if you use a timestep about 10x
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advised.
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larger than you would normally use for dynamics simulations.
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:line
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:line
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